Determinaciones de paleointensidad en una secuencia volcánica en el Cáucaso menor, Georgia
- Ana Caccavari 1
- Avto Goguitchaichvili 1
- Manuel Calvo-Rathert 2
- Juan Morales 1
- Miguel Cervantes Solano 1
- Goga Vashakidze 3
- He Huaiyu 4
- V. A. Lebedev 5
- Néstor Vegas 6
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1
Universidad Nacional Autónoma de México
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2
Universidad de Burgos
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3
Tbilisi State University
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4
Chinese Academy of Sciences
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5
Institute of Geology of Ore Deposits Petrography Mineralogy and Geochemistry
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Institute of Geology of Ore Deposits Petrography Mineralogy and Geochemistry
Moscú, Rusia
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6
Universidad del País Vasco/Euskal Herriko Unibertsitatea
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Universidad del País Vasco/Euskal Herriko Unibertsitatea
Lejona, España
ISSN: 2007-9656
Year of publication: 2016
Volume: 6
Issue: C02
Pages: 1-7
Type: Article
More publications in: Latinmag Letters
Abstract
We report forty-six successful absolute geomagnetic paleointensity determinations from a Pleistocenelava sequence composed of 39 successive flows in the Djavakheti Highland (Lesser Caucasus, Georgia).Available radiometric and paleomagnetic data suggest that either the lower 36 flows of the sequence mighthave been emitted between the normal-polarity Reunion and Olduvai chrons and the upper three flows afterthe Olduvai chron, or the whole sequence might have been emplaced in a short time between the Olduvaichron and 1.73 + 0.03 Ma (Caccavari et al., 2014).Paleointensity studies were performed using a Thellier type double heating method. Samples selection wasmainly based on uni-vectorial remanent magnetization, thermal stability and domain size of the samples. Flow-mean paleointensity values range from 16 ± 7.3 to 56.7 ± 15.8 µT, and corresponding virtual dipolemoments range from 2.25 ± 1.03 to 8.44 ± 2.71 x 1022 Am2.Two flows yield rather low absolute intensity suggesting a transitional regime. These flows are located neara possible discontinuity in the sequence, suggesting the onset of the Matuyama-Olduvai polarity transition,which does not appear on the directional record. This supports the interpretation of a long hiatus in volcanicactivity after the emission of the 36 lower flows of the sequence. sParts of the Virtual Dipole Momentsobtained in the present work are similar to those obtained in the same region in another lava flow sequenceof similar age.
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